Diya
Sign in to saveAlso known as WASP-72
WASP-72 (also known as CD-30 1019 and officially named Diya) is the primary of a binary star system. It is an F7 class dwarf star, with an internal structure just on the verge of the Kraft break. It is orbited by a planet, WASP-72b. The age of WASP-72 is younger than the Sun at 3.55 billion years.
In the Vinony graph
Vinony's link graph records 109 inbound references to Diya, and connects out to list of stars in Fornax, HD 20781 and year.
Vinony files it under Binary stars, Durchmusterung objects and Fornax.
Vinony links it to 5 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- *
- Distance
- 1,365 light-years
- Redshift
- z = 0.000124627311949288
- Coordinates
- RA 41.0400° · Dec -30.1690°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Fornax
- Distance from Earth
- 434.754
- Radius
- 2.66
- Mass
- 1.03
Show 16 more facts
- catalog code
- TOI-264
- effective temperature
- 5773.47
- parallax
- 2.305
- apparent magnitude
- 10.846672
- radial velocity
- 35.35
- epoch
- J2000.0
- surface gravity
- 6780
- name
- Diya
- luminosity
- 6.5762944
- right ascension component of proper motion
- 7.614
- declination component of proper motion
- -7.673
- age estimated by a dating method
- 5
- right ascension
- 41.04004000976001
- declination
- -30.16904546173
- metallicity
- -0.085
- spectral class
- G2IV
via Wikidata · CC0
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Encyclopedic overview
2 sectionsContents
- Planetary system
- References
WASP-72 (also known as CD-30 1019 and officially named Diya) is the primary of a binary star system. It is an F7 class dwarf star, with an internal structure just on the verge of the Kraft break. It is orbited by a planet, WASP-72b. The age of WASP-72 is younger than the Sun at 3.55 billion years.
The primary seems to have UV-opaque matter in the line-of-sight, which may originate from atmosphere escaping from WASP-72b or from an unknown object in the interstellar medium. WASP-72 was named Diya in 2019.
Excerpted from Wikipedia’s “Diya” article, available under the CC BY-SA 4.0 licence.